The 1998, 1999, 2000 and 2001 statistics shows that the Klet' Observatory was the second world most prolific site producing astrometry of PHAs published in Minor Planet Electronic Circulars, the LINEAR project was the first.

In 2002 we received a new MPC code 246 Kleť Observatory-KLENOT for our new 1.06-m KLENOT Telescope and started NEO follow-up astrometry up to limiting magnitude V = 22.